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Linear stability of Schwarzschild spacetime subject to axial perturbations

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abstract

In this paper, we address the issue of linear stability of Schwarzschild space- time subject to certain axisymmetric perturbations. In particular, we prove that associ- ated solutions to the linearized vacuum Einstein equations centered at a Schwarzschild metric, with suitably regular initial data, decay to a linearized Kerr metric. Our method employs a complex line bundle interpretation applied to a connection-level object, allow- ing for direct analysis of this connection-level object by the linearized Einstein equations, in contrast with the recent breakthrough of Dafermos-Holzegel-Rodnianski.

fields

gr-qc 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

Nonlinear stability of subextremal Kerr black holes

gr-qc · 2026-06-26 · unverdicted · novelty 8.0

Proves global nonlinear stability of subextremal Kerr black holes, with solutions settling to a nearby Kerr member at rate O(t_*^{-2-ε_K}) from initial data with O(r^{-1-ε0}) decay.

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  • Nonlinear stability of subextremal Kerr black holes gr-qc · 2026-06-26 · unverdicted · none · ref 39 · internal anchor

    Proves global nonlinear stability of subextremal Kerr black holes, with solutions settling to a nearby Kerr member at rate O(t_*^{-2-ε_K}) from initial data with O(r^{-1-ε0}) decay.